A 6 dimensional $(Z_{2})^3$ symmetric model with warped physical space
| dc.creator | Sahabandu, Chetiya | |
| dc.creator | Suranyi, Peter | |
| dc.creator | Vaz, Cenalo | |
| dc.creator | Wijewardhana, L. C. Rohana | |
| dc.date | 2008-04-14 | |
| dc.date | 2008-04-18 | |
| dc.date.accessioned | 2026-07-07T11:33:35Z | |
| dc.date.available | 2026-07-07T11:33:35Z | |
| dc.description | The Randall-Sundrum model is studied in 6 dimension with AdS$_4$ or dS$_4$ metric in the physical 4 dimensional space. Two solutions are found, one with induced 5-dimensional gravity terms added to the induced cosmological constant terms. We study the graviton modes in both solutions by transforming the mass eigenvalue equation to a Schrodinger equation with a volcano potential. The spectrum of gravitational excitations depends on the input parameters of the theory, the six dimensional and the effective four-dimensional cosmological constants. The model gives a physically acceptable spectrum if the 4 dimensional cosmological constant is sufficiently small. | |
| dc.description | 14 pages, 3 tables, 2 references added | |
| dc.identifier | https://arxiv.org/abs/0804.2066 | |
| dc.identifier | http://arxiv.org/abs/0804.2066 | |
| dc.identifier | J.Phys.A41:304012,2008 | |
| dc.identifier | doi:10.1088/1751-8113/41/30/304012 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197947 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | A 6 dimensional $(Z_{2})^3$ symmetric model with warped physical space | |
| dc.type | text |